Jean Tarde and Jan Smogulecki carried out sunspot observations in the 1610s and 1620s at the dawn of the telescopic era. We analysed their original observational records to revise their sunspot-group numbers in the existing database. In this study, we provide a new counting as a basis for future scientific discussions. Furthermore, we compared Smogulecki’s sunspot observations with those of Scheiner and Schönberger on the same observation days. We also detected a big sunspot group on 2 – 3 February 1622 in Smogulecki’s sunspot drawings and estimated its area to be approximately 1600 millionths of the solar disc. In addition, we measured the sunspot positions in Tarde’s and Smogulecki’s sunspot drawings to construct a butterfly diagram for t...
The International Sunspot Number is used as a measure of the level of solar activity in many importa...
Context. Sunspots have been observed since Galileo Galilei invented the telescope. Later, sunspot d...
The sunspot number is “arguably the most intensively studied time series in astrophysics ” [Charbonn...
• Financiación Open Access por Acuerdo CRUE-CSIC con Springer NatureJean Tarde y Jan Smogulecki real...
We have examined the more than 1100 drawings of the solar disk made by the German astronomy amateur ...
Sunspot observations are available in fairly good numbers since 1610, after the invention of the tel...
Samuel Heinrich Schwabe made 8486 drawings of the solar disc with sunspots in the period from 1825 N...
Abstract Context: The group sunspot number (GSN) series constitute the longest instrumental astronom...
Kodaikanal Solar Observatory (KoSO) possesses one of world's longest and homogeneous records of suns...
Abstract Aims: Sunspot number series are composed from observations of hundreds of different observe...
Visual sunspot observations are at the base of the single longest scientific record ofsolar activity...
Abstract. At the XIIth Hvar Astrophysical Colloquium in 2012, we reviewed the progress of an effort ...
Aims. Sunspot number series are composed from observations of hundreds of different observers that r...
Aims. Digital images of observations printed in the books Rosa Ursina sive solis and Prodromus pro s...
Sunspots have a diameter of about 37,000 km and appear as dark spots within the photosphere, the out...
The International Sunspot Number is used as a measure of the level of solar activity in many importa...
Context. Sunspots have been observed since Galileo Galilei invented the telescope. Later, sunspot d...
The sunspot number is “arguably the most intensively studied time series in astrophysics ” [Charbonn...
• Financiación Open Access por Acuerdo CRUE-CSIC con Springer NatureJean Tarde y Jan Smogulecki real...
We have examined the more than 1100 drawings of the solar disk made by the German astronomy amateur ...
Sunspot observations are available in fairly good numbers since 1610, after the invention of the tel...
Samuel Heinrich Schwabe made 8486 drawings of the solar disc with sunspots in the period from 1825 N...
Abstract Context: The group sunspot number (GSN) series constitute the longest instrumental astronom...
Kodaikanal Solar Observatory (KoSO) possesses one of world's longest and homogeneous records of suns...
Abstract Aims: Sunspot number series are composed from observations of hundreds of different observe...
Visual sunspot observations are at the base of the single longest scientific record ofsolar activity...
Abstract. At the XIIth Hvar Astrophysical Colloquium in 2012, we reviewed the progress of an effort ...
Aims. Sunspot number series are composed from observations of hundreds of different observers that r...
Aims. Digital images of observations printed in the books Rosa Ursina sive solis and Prodromus pro s...
Sunspots have a diameter of about 37,000 km and appear as dark spots within the photosphere, the out...
The International Sunspot Number is used as a measure of the level of solar activity in many importa...
Context. Sunspots have been observed since Galileo Galilei invented the telescope. Later, sunspot d...
The sunspot number is “arguably the most intensively studied time series in astrophysics ” [Charbonn...